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Search: L773:0035 8711 OR L773:1365 2966 OR L773:1745 3925 OR L773:1745 3933 > (2020-2024) > A precursor plateau...

A precursor plateau and pre-maximum [O ii] emission in the superluminous SN2019szu : a pulsational pair-instability candidate

Aamer, Aysha (author)
Nicholl, Matt (author)
Jerkstrand, Anders, 1978- (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
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Gomez, Sebastian (author)
Oates, Samantha R. (author)
Smartt, Stephen J. (author)
Srivastav, Shubham (author)
Leloudas, Giorgos (author)
Anderson, Joseph P. (author)
Berger, Edo (author)
de Boer, Thomas (author)
Chambers, Kenneth (author)
Chen, Ting-Wan (author)
Galbany, Lluís (author)
Gao, Hua (author)
Gompertz, Benjamin P. (author)
González-Bañuelos, Maider (author)
Gromadzki, Mariusz (author)
Gutiérrez, Claudia P. (author)
Inserra, Cosimo (author)
Lowe, Thomas B. (author)
Magnier, Eugene A. (author)
Mazzali, Paolo A. (author)
Moore, Thomas (author)
Müller-Bravo, Tomás E. (author)
Pursiainen, Miika (author)
Rest, Armin (author)
Schulze, Steve, 1980- (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Smith, Ken W. (author)
Terwel, Jacco H. (author)
Wainscoat, Richard (author)
Young, David R. (author)
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 (creator_code:org_t)
2023
2023
English.
In: Monthly notices of the Royal Astronomical Society. - 0035-8711 .- 1365-2966. ; 527:4, s. 11970-11995
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We present a detailed study on SN2019szu, a Type I superluminous supernova at z = 0.213 that displayed unique photometric and spectroscopic properties. Pan-STARRS and ZTF forced photometry show a pre-explosion plateau lasting ∼40 d. Unlike other SLSNe that show decreasing photospheric temperatures with time, the optical colours show an apparent temperature increase from ∼15 000 to ∼20 000 K over the first 70 d, likely caused by an additional pseudo-continuum in the spectrum. Remarkably, the spectrum displays a forbidden emission line (likely attributed to λλ7320,7330) visible 16 d before maximum light, inconsistent with an apparently compact photosphere. This identification is further strengthened by the appearances of [O III] λλ4959, 5007, and [O III] λ4363 seen in the spectrum. Comparing with nebular spectral models, we find that the oxygen line fluxes and ratios can be reproduced with ∼0.25 M⊙ of oxygen-rich material with a density of ∼10−15 g cm−3⁠. The low density suggests a circumstellar origin, but the early onset of the emission lines requires that this material was ejected within the final months before the terminal explosion, consistent with the timing of the precursor plateau. Interaction with denser material closer to the explosion likely produced the pseudo-continuum bluewards of ∼5500 Å. We suggest that this event is one of the best candidates to date for a pulsational pair-instability ejection, with early pulses providing the low density material needed for the formation of the forbidden emission line, and collisions between the final shells of ejected material producing the pre-explosion plateau.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

stars: massive
supernovae: general
supernovae: individual: SN2019szu
transients: supernovae

Publication and Content Type

ref (subject category)
art (subject category)

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